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Surface of Titania

The surface of Titania is like many icy moons. It appears to be changed for it does not have many craters. Instead it has grooves similar to those found on Ganymede. These grooves extend for m
any kilometers over the surface. The presence of grooves indicates that there has been activity in the interior of Titania in the past.

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Miranda was discovered by G. Kuiper in 1948. Miranda one of the smallest icy moons, and is as wide as the distance from Los Angeles to San Francisco. The surface features of this moon are hard to see in...more

The surface of Miranda is very unusual. It is not like any other moon in the solar system. Miranda has many craters but also very big grooves. These show that there has been activity inside Miranda in...more

The surface of Oberon is like many icy moons. It appears to be changed for it does not have many craters. Instead it has grooves similar to those found on Ganymede. These grooves extend for ma ny kilometers...more

The surface of Oberon is like many icy moons. It appears to be changed for it does not have many craters. Instead it has grooves similar to those found on Ganymede. These grooves extend for ma ny kilometers...more

Titania was discovered by W. Herschel in 1787. Titania is about as wide as the state of California is long. The surface features of this moon are hard to see in this image. The surface suggests that Titania...more

The surface of Titania is like many icy moons. It does not have many craters. Instead it has grooves similar to those found on Ganymede. These grooves extend for many kilometers over the surface. ...more